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| author | tlatorre <tlatorre@uchicago.edu> | 2019-01-29 13:20:59 -0600 |
|---|---|---|
| committer | tlatorre <tlatorre@uchicago.edu> | 2019-01-29 13:20:59 -0600 |
| commit | 10502e7ed56c9cce707fcf027e9ba5a9e2695303 (patch) | |
| tree | 4189dbeb9c31fde304fa7d77fd7eb5beff932c9b /src | |
| parent | c79b3cf71e2e22f704e724e0c5ecb156550ac32e (diff) | |
| download | sddm-10502e7ed56c9cce707fcf027e9ba5a9e2695303.tar.gz sddm-10502e7ed56c9cce707fcf027e9ba5a9e2695303.tar.bz2 sddm-10502e7ed56c9cce707fcf027e9ba5a9e2695303.zip | |
normalize delta ray charge by total range
This is so that in the future if we only integrate over the path in the PSUP we
don't overestimate the Cerenkov light from delta rays.
Diffstat (limited to 'src')
| -rw-r--r-- | src/likelihood.c | 6 |
1 files changed, 2 insertions, 4 deletions
diff --git a/src/likelihood.c b/src/likelihood.c index 8e12f57..aab4ede 100644 --- a/src/likelihood.c +++ b/src/likelihood.c @@ -404,8 +404,6 @@ static void integrate_path_shower(particle *p, double *x, double *pdf, double T0 n_d2o = get_index_snoman_d2o(wavelength0); n_h2o = get_index_snoman_h2o(wavelength0); - double range = x[n-1] - x[0]; - for (i = 0; i < n; i++) { pos[0] = pos0[0] + x[i]*dir0[0]; pos[1] = pos0[1] + x[i]*dir0[1]; @@ -416,8 +414,8 @@ static void integrate_path_shower(particle *p, double *x, double *pdf, double T0 t = x[i]/SPEED_OF_LIGHT + l_d2o*n_d2o/SPEED_OF_LIGHT + l_h2o*n_h2o/SPEED_OF_LIGHT; qs[i] = get_expected_charge_shower(p, pos, dir0, pmts[pmt].pos, pmts[pmt].normal, PMT_RADIUS, q_indirects+i, n_d2o, n_h2o, l_d2o, l_h2o, &q_delta_ray, &q_indirect_delta_ray); - qs[i] = qs[i]*pdf[i] + q_delta_ray/range; - q_indirects[i] = q_indirects[i]*pdf[i] + q_indirect_delta_ray/range; + qs[i] = qs[i]*pdf[i] + q_delta_ray/p->range; + q_indirects[i] = q_indirects[i]*pdf[i] + q_indirect_delta_ray/p->range; ts[i] = t*qs[i]; ts2[i] = t*t*qs[i]; } |